X-ray Beamline Design 2012cheiron2012.spring8.or.jp/text/Lec5_S.Goto.pdf · G x y z π π π π π...
Transcript of X-ray Beamline Design 2012cheiron2012.spring8.or.jp/text/Lec5_S.Goto.pdf · G x y z π π π π π...
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X-ray Beamline Design 1
X-ray Monochromator
Shunji GotoSPring-8/JASRI
September 25, 2012
Cheiron School 2012
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Outline
1. Introduction2. Light source3. X-ray Monochromator
Fundamental of Bragg reflectionDynamical theoryDuMond diagram ~ extraction of x-rays from SRDouble crystal monochromatorCrystal cooling
4. Example of beamlines at SPring-85. Summary
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SR
Experimental station
Exp. hallRing tunnel
Front-end
Beamline structureBeamline = “Bridge” between light source & experimental station
Transport and processing of photonsphoton energy, energy resolution,beam size, beam divergence, polarization,..
Light source
Monochromator, mirror
shutter, slit
pump,..
Vacuumprotection of ring vacuum and beamline vacuum
Radiation safety
Shielding and interlock
Bending magnet
Insertion device
Shielding hutch
Optics & transport
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Light sources & X-ray optics
- White or monochromatic
- Energy range
- Energy resolution
- Flux & flux density
- Beam size at sample (micro beam?,...)
- Beam divergence/convergence at sample (Resolution in k-space)
- Higher order elimination w/ mirror
- Polarization conversion
- Spatial coherency
....
Check points to be considered for your SR application:
Light source, monochromator, mirror,
and other optical devices and components
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BL classification (energy region)
Photon energy (eV)
IR
101 103 104 105
Undulator
Bending magnet
Wiggler
SX-PES
102
Earth,..HP/HT
Inelastic
Inelastic
SAXS
PX
XAFSPowder XRD
HP/HT XRD
NRS
SAXS
SX-MCD
PEEM
HX-PES
HXSXIR
100
Visible ~ UV~
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BL classification (energy resolution)
Undulator
Bending magnet
White
Earth,..HP/HT
10-7 10-5 10-3
XAFSSAXS
XAFS
SAXS
PX
PX
Inelastic
NRSHX-PES
Topograph
Topograph
Surface ・interface XRF
Powder XRD
Wiggler Inelastic
Microbeam, imagingXMCD
Imaging
HP/HT XRD
Single crystal XRD
Energy resolution (ΔE/E)
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Light sources (1)
Bending magnet or insertion devices ?
Bending magnet:for wide energy range, continuous spectrum
for wide beam application for large samples
Undulator (major part of 3GLS beamline):for high-brilliance beam
for micro-/ nano-focusing beam
Wiggler:for higher energy X-rays > 100 keV. 1012
1014
1016
1018
1020
1022
Bril
lianc
e (p
h/s/
mm
2/m
rad2
/0.1
% B
.W.)
100 101 102 103 104 105 106
Photon energy (eV)
Brilliance for SPring-8 casePower, brilliance, flux density, partial flux,.. can be calculated using code.
e.g. “SPECTRA” by T. Tanaka & H. Kitamura
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Light sources (2)Angular divergence and band width
Core part we need
Bending magnet
Undulatorc
r λλ
γσ 1597.0≈′
nNK
N un
r21
21
2
2+=≈′ γλ
λσ
nNEE 1
≈Δ
SPring-8 in-vacuum undulator
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γψ 1≈vPower distribution
consth ≈ψ
γψ 1≈vγψ Kh ≈
K: deflection parameter (K= 0.5~2.5)
]A[]rad[]m[]T[]GeV[27.1]kW[ 22tot IRBEP φ= ]A[]m[]T[21]GeV[27.1]kW[ 20
2tot ILBEP =
Total power
E= 8 GeV, I= 0.1 A, B= 0.68 T, R= 39.3 m Ptot= 0.15 kW/mrad
B0= 0.87 T, L= 4.5 mPtot= 14 kW
]m[ArcL ( )uzB λπ2sin220
Light sources (3)
Bending magnet Undulator
Kilowatt of SR power mostly eliminated before/by monochromator
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X-ray MonochromatorX-ray monochromator is key component for SR experiments:
length gauge for structure analysis,energy gauge for spectroscopy,...
Principle of x-ray monochromator
Photon energy tuning Bragg’s law
Energy resolution source divergence, Darwin width,..
Flux (throughput) related to Darwin width
Understanding the dynamical theory for large & perfect crystal
Practical of the monochromator
Double-crystal monochromator for fixed-exit
Single-bounce monochromator is for limited case
Crystal cooling
High heat load depending on light source
Mechanical engineering issues
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λθ md =Bsin2
θ θ d
dsinθ dsinθ
hKKQ =−= 0s
Bragg’s law in real space Laue condition (Kinematical)in reciprocal space
Reciprocal lattice vector h- Normal to net plane- Length = 1/d
1) Phase matching on the single net plane by mirror-reflection condition.
2) Phase matching between net planes.
net plane (spacing d)
Reciprocal lattice vector h
Scattering vector Q
Scattered wave Ks
Incident wave K0 θ θ
Bragg reflection
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Ewald sphere
Ewald sphere:
When a reciprocal lattice point is on the Ewald sphere, Bragg reflection occurs.
Reciprocallattice points
0K
SK01 KRadius == λ
h
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Top view
Side view
[100]
[011]
[010]
[001]
(400)
(511)
(111) : 3.1356 Ǻ(311) : 1.6375 Ǻ
(400) : 1.3578 Ǻ
(511) : 1.0452 Ǻ
a
a
d-spacing
(111) (311)
222 lkh
ad++
=
Miller indices and d-spacing for silicon
a = 5.431Å
Diamond : a = 3.567Å
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( ) ( ) ( )∑ ⋅=j
jj iEfF rhhh π2exp,
( ) ( ) ( ){ }∑ ++=j
jjjj lzkyhxiEfF π2exp,hh
lkh ,, Mixture of odd and even numbers0=F
All odd, or, all even numbers, and m: integer,
mlkh 4=++ fF 8= 8 atoms in phase
14 ±=++ mlkh ( ) fiF ±= 14
24 ±=++ mlkh 0=F
Half contribute with phase shift ±π /2
lkh ,,
Half cancel with π
For diamond structure
Structure facrtor Sum of atomic scattering with phase shift in the unit cell
Position of atoms in the unit cell for diamond structure
(xj, yj, zj) =
(0, 0, 0)1, (1/4, 1/4, 1/4)2,
(1/2, 1/2, 0)3, (3/4, 3/4, 1/4)4,
(0, 1/2, 1/2)5, (1/4, 3/4, 3/4)6,
(1/2, 0, 1/2)7, (3/4, 1/4, 3/4)8
1
2zy
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5
6
7 8Atomic scattering factor
Crystal structure factor for diamond structure
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(400), (220),...
All in phase
[100]
[011]
(400)
(511)
a
(111) (311)
(111), (311),... Half contribute with phase shift ±π /2
(200)
(011), (200),...
Half cancel with π
Forbidden reflection
(011)
( ) fiF ±= 14fF 8=
0=F
Crystal structure factor for diamond structure
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X-ray monochromator using perfect crystal
Perfect single crystal: silicon, diamond,..
0
20
40
60
80
100
120
0 5 10 15 20 25 30Bragg angle (deg)
Pho
ton
ener
gy (k
eV)
Si 111 refl.
Si 311 refl.
Si 511 refl.
e.g. for SPring-8 standard DCM
Bragg angle: 3~27°
Photon energy tuning:
Crystal & lattice plane
Bragg angle range
Bsin][23984.12]keV[
θÅhkldE =
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( ) ( ) 22 QQ GFII e ⋅=
Peak intensity 2xN
FWHM xx NNh 1~8858.0≈Δ
Crystal size becomes larger narrower & higher, approaching delta function
( ) ( )( )( )
( )( )
( )llN
kkN
hhNG zyx
ππ
ππ
ππ
2
2
2
2
2
22
sinsin
sinsin
sinsin
⋅⋅=QLaue function:
h, k, l: integer Intense peaks(hkl) reflection
3-dim. Periodic structure
0
20
40
60
80
100
-1.5 -1 -0.5 0 0.5 1 1.5 2 2.5
120
( )( )h
hNxπ
π2
2
sinsin
h
One-dim. Laue function, Nx= 10
Kinematical X-ray diffraction
NxNy
Nz
cba zyx nnn ++
Unit cell
3-dimensional periodic structure of unit cell with number Nx, Ny, NzTotal scattering intensity becomes:
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Dynamical theoryTwo-wave approximation
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Kinematical to dynamical theory
“Large & perfect” single crystal:1) Multiple scattering w/ h & -h reflection2) Extinction
(Diffraction by “finite” number of net planes)
Kinematical diffraction is invalid Dynamical theory must be applied.
Net plane
Incident wave Diffracted wave
Extinction
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Fundamental equation
h, g,... : Reciprocal lattice points
Eh, Eg : Fourier components of electric field
K0 : Incident wave vector in vacuum
kh : Wave vectors in the crystal
χh : Fourier components of the polarizability (Negative values, 10-6~10-5)
P= (eh・eg) : Polarization factor between h and g waves
kh= k0 + h : Momentum conservation
Fundamental equation is derived
using Maxwell’s equations and introducing Bloch wave
for 3-dimensional periodic medium (= perfect single crystal):
( )∑ ⋅=− −g
gghghhh EE
KKk eeχ2
0
20
2
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Two-wave approximation
: Fourier components of the polarizability
(Negative values, 10-6~10-5)
: Polarization factor ( )
Fundamental equation is reduced to the equation for
two waves of incidence and “one” intense diffraction
( )∑ ⋅=− −g
gghghhh EE
KKk eeχ2
0
20
2 ( ) hhEPEEKKk
−+=− χχ 0002
0
20
20A
( ) hhhh EEPEKKk
002
22
B χχ +=−
hh −χχχ ,,0
( )hP ee ⋅= 0 BPP θπσ 2cos:,1: ==
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Two-wave approximation
( ) hhEPEEKKk
−+=− χχ 0002
0
20
20A
( ) hhhh EEPEKKk
002
22
B χχ +=−
hE0χ
00Eχ
0Ehχ
Scheme of self-consistent wave field
hhE−χ0E⇒
hE⇒0E
hE
( )( ) 40222220 KPkk hhh −=−− χχkk( ) 2002 1 Kk χ+=
Using two equations, we obtain following secular equation:
h
h−
Secular equation
k : Mean wave number in the crystal
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Boundary condition of wave vector
Tangential component of wave vector must be continuous.
Incident wave in vacuum
Refracted wave in the crystal
Bragg reflection in the crystal
Reflected wave in the crystal
Reflected wave in vacuum
K0 Kh
k0 kh
Vacuum Crystal
We must consider connections of waves from vacuum into the crystal and from the crystal to vacuum, to solve the equations.
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Laue case and Bragg case
K0 Kh
n
K0 Kh
n
Laue case(Transmission geometry)
Bragg case(Reflection geometry)
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Asymmetry ratio
h
bγγ 0=
nK ⋅= 00 ˆγ
nKhh ⋅= ˆγ
Laue case: b>0
Symmetric Laue case: b= 1
Bragg case: b< 0
Symmetric Bragg case: b= -1
K0 Kh
n
n: normal vector to the surface
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Dispersion surface( )( ) 40222220 KPkk hhh −=−− χχkk
Two dispersion surfaces show the gap near Bragg condition.
h
kh
k0 O
H
Reciprocal spaceReal space
Secular equation is quartic equation, and it gives four-point solution on the n-vector,producing the dispersion surfaces.
n-Laue
n-Bragg
K0 Kh
n
K0 Kh
n
Laue case
Bragg case
0K
0K
Laue case
Bragg case
kh= k0 + h
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Deviation from Bragg condition
Excitation errorGeometrical deviation ζ0 from Bragg condition:
Distance between Ewald sphere and the reciprocal lattice point.
ζ0 is positive when H is inside the Ewald sphere (by S. Miyake).
O
H
0K
SK 0ζ
h
( )0
20
0 22
Kh+⋅
−≈hKς
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Normalized deviation parameter W
For symmetric Bragg case, sigma polarization:
Parameter W is related to the gap between two dispersion surfaces
and total reflection occurs at –1
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Sign of deviation parameter W
Angle deviation at fixed energy
direction change of wave vector
Energy deviation at fixed angle
length change of wave vector
h h0W
00 →> WEE
0K0K
0EE =
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Movement of tie point
(3) Higher angleW> 1
h
kh
k0 O
H
K0 Kh
Vacuum
Crystal
h
kh
k0 O
H
K0 Kh
Total reflection
(1) Lower angleW< -1
(2) Near Bragg condition-1< W< 1
h
kh
k0 O
H
K0 Kh
Dominant branch for thick Bragg-case crystal is close to O-sphere.
Tie point moves by changing the incident angle
at fixed photon energy (wavelength).
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Calculation of polarizability
hihrh χχχ +=
For diamond structure
( ) Mc
ehr effv
r −′+−= 02
8π
λχ
M
c
ehi efv
r −′′−= 82
πλχ
( )fZv
r
c
er ′+−= 8
2
0 πλχ
fv
r
c
ei ′′−= 8
2
0 πλχ
mlkh 4=++
14 ±=++ mlkh
0=== lkh
( )( ) Mc
ehr effiv
r −′++−= 02
14π
λχ
( ) Mc
ehi efiv
r −′′+−= 142
πλχ
χh: Fourier component of polarizabilityproportional to the structure factor
vc: unit cell volume
( )EFv
r
c
eh ,
2
hπ
λχ −=
( ) ( )Effhr ′+⇔ h0χ
Atomic form factor + real part of anomalous factor
( )Efhi ′′⇔χImaginary part of anomalous factor
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Amplitude ratio
From the solution of the fundamental equations, we obtain the ratio r = Eh/E0 ( reflection coefficient)as a function of parameter W.
For Bragg case, no absorption, and thick crystal:
( ) )1(1200
−−−−==−
WWWPP
EEr
h
hr
h
h
χχ
γγ
Total reflection
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( ) )1(1 22 −−−= WWWR
hEEW
χχθθθ 1sin22sin 0B
2B ⎟
⎠⎞
⎜⎝⎛ +
Δ+Δ=
W: deviation parameter for s-polarization, symmetrical Bragg case
Angular deviation
Energy deviation
Geometry for symmetrical Bragg case
net plane
K0
Bθ SurfaceBθ
Khθθ Δ+Bθθ Δ+B
Refraction
Total reflection region
Darwin curve (intrinsic reflection curve for monochromatic plane wave)for Bragg case, no absorption, and thick crystal:
Reflectivity (Darwin curve)
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Darwin curve
For Bragg case, no absorption, and thick crystal:
0
0.2
0.4
0.6
0.8
1
1.2
-5 -4 -3 -2 -1 0 1 2 3 4 5
W
Ref
lect
ivity
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Reflectivity with absorption
- symmetrical Bragg case, - s-polarization, - thick crystal
12 −−= LLR
( ) ( )2
2222222
1
41
κ
κκ
+⎭⎬⎫
⎩⎨⎧ −++−−++
=gWgWgW
L
rh
hi
rh
igχχ
κχχ
== ,0hr
rEEW
χχθθθ 1sin22sin 0B
2B ⎟
⎠⎞
⎜⎝⎛ +
Δ+Δ=
Reflectivity
Note: No absorption curveDarwinRg →⇒== 0,0 κ
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Reflectivity curve for silicon
・Width of 0.1~100 µrad・Peak ~1 with small absorption
回折幅
0
0.2
0.4
0.6
0.8
1
-100 -50 0 50 100Δθ (µrad)
Ref
lect
ivity
Si 111 refl. 10 keV
Si 333 refl. 30 keV
Examples for symmetrical Bragg case, with absorption, s-polarization and thick crystal:
Si 111 refl., 10 keV
( )( )i
i
i
r
i
r
+×−=
+×−=
×−=
×−=
−
−
−
−
11030.7
11066.3
1048.1
1078.9
8_111
6_111
70
60
χ
χ
χ
χ
( )( )i
i
i
r
i
r
+×−=
+×−=
×−=
×−=
−
−
−
−
11087.7
11024.2
1075.1
1007.1
10_333
7_333
90
60
χ
χ
χ
χ
Si 333 refl., 30 keV
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Effective band width
2Darwin
2Bcot θθ Δ+Ω=
ΔEE
Energy resolution
B2sin θ
χhrEE
≈Δ
Angular width(Darwin width)
( )hFhr ∝=ΔB
Darwin 2sin2
θχ
θ
Gaussian approximation for both light source and reflection curve
EEΔRelative energy
1−=W 1=W
Incident angleBθ θ
Darwin width
Shift by refraction
Kinematical Bragg condition
Bcotθ−Slope:
EEΔRelative energy
Incident angle θ
Energy resolution
Effective band width
Light source divergence φ
Light source
ΔW= 2
The diagram helps to understand how we can extract x-rays from SR source.
DuMond (angle-energy) diagram
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Source divergence and diffraction width
Divergence of undulator radiation ~ diffraction width
- Bending magnet
μrad60≈′rσ
- Undulator (N= 140)μrad5r ≈′σ
For SPring-8 case:
- Undulatorωλ
λγ
σh
11597.0 ∝≈′c
r
- Bending magnet
Natural divergence
ωλλσ
h
12
∝≈′u
r N
103
0 20 40 60 80 100
Photon energy (keV)
FWH
M (µ
rad)
102
101
100
10-1
Bending magnet
Undulator
Si 111 refl.
Si 311 refl.
Si 511 refl.
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Energy resolution
For usual beamline : ΔE/E=10-5~10-3
22Bcot ωθ +Ω=
ΔEE Ω: source divergence,
ω: diffraction width
Angle-energy diagram(DuMond diagram)
φ
Pho
ton
ener
gy
Light source distribution
Δθ, φ
Acceptance by crystal
Resolution
10-5
10-4
10-3
10-2
0 20 40 60 80 100Photon energy (keV)
ΔE/E
BM & Si 111 refl.
BM & Si 311 refl.
BM & Si 511 refl.
Undulator & Si 111 refl.
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DuMond diagram: undulator & DCMSPring-8 standard undulator
(λu= 32 mm, N= 140, K= 1.34, E1st= 10 keV)
+ DCM (Si 111 refl.)
10 keV (1st) 30 keV (3rd) 50 keV (5th)
Wider slit increases unused photons (power) on the monochromator !
Intensity distribution of
undulator
200
ΔE(e
V)
-50 500φ (μrad)
-200
0
600
ΔE(e
V)
-50 500φ (μrad)
-600
0
1000
ΔE(e
V)
-50 500φ (μrad)
-1000
0
φ
Acceptance by crystal
DE/
E= 2
x10-
4
50 μrad Undulator radiation: ( )2220 21 φγ++= KEE
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DuMond diagram: undulator & DCM
SPring-8 standard undulator + 20 μrad slit + Si 111 DCM10-keV photons 1.3x10-4
100 μrad
ΔE/E
= 5x
10-4
-3
-2
-1
0
1
2
3
00.20.40.60.81Intensity (arb. units)
Rel
ativ
e en
ergy
(eV
)FWHM= 1.3 eV
Acceptance by Si 111 DCM
Undulator radiation
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Improvement of energy resolution
(A) Collimation using slit (B) Collimation using pre-opticsw/ collimation mirror, CRL,..
(C) Additional crystalw/ (+,+) setting
(D) HR monochromator of π/2 reflection (~meV)
Pho
ton
ener
gy
Angle
ResolutionP
hoto
n en
ergy
Angle
Resolution
(B)~(D): restriction on photon energy
Pho
ton
ener
gy
Angle
Resolution
Light source distribution
Acceptance by crystal
Pho
ton
ener
gy
Angle
Resolution
Slit width
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Improvement of energy resolution(C) Additional crystal w/ (+,+) setting
HXPES
Si 111 DCM Si nnn channel-cut mono.
Si 333 refl. for 6 keV
Si 555 refl. for 10 keV
40 μrad
ΔE/E
= 5x
10-5
-100
-80
-60
-40
-20
0
20
40
60
80
100
00.20.40.60.81
Intensity (arb. units)
Rel
ativ
e en
ergy
(meV
)
-100
-80
-60
-40
-20
0
20
40
60
80
100
00.20.40.60.81
Intensity (arb. units)
Rel
ativ
e en
ergy
(meV
)
FWHM= 45 meV
FWHM= 18 meV
Phot
on e
nerg
y
Angle
Resolution
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Improvement of energy resolution
Si 111 DCM Si nnn back-scattering mono.
Si 999 refl. for 17.8 keV
Si 11 11 11 refl. for 21.7 keV
20 μrad
ΔE/E
= 5x
10-7
(D) HR monochromator of ~π/2 reflection (~meV) Inelastic scattering
Phot
on e
nerg
y
Angle
Resolution
-4
-3
-2
-1
0
1
2
3
4
00.20.40.60.81
Intensity (arb. units)
Rel
ativ
e en
ergy
(meV
)
-4
-3
-2
-1
0
1
2
3
4
00.20.40.60.81Intensity (arb. units)
Rel
ativ
e en
ergy
(meV
)
FWHM= 2.0 meV
FWHM= 0.87 meV
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Photon flux after monochromatorPhoton flux (throughput) after monochromator can be estimated using effective band width:Photon flux (ph/s) =
Photon flux from light source (ph/s/0.1%bw)
x 1000
x Effective band width of monochromator
Throughput is estimated by overlapped area.
Note difference from energy resolution.
Pho
ton
ener
gy Light source
distribution
Angle
Effective band width
Acceptance by crystal
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Effective band width
( ){ }λλχ fdf hklhr ′+∝ )(02
Independent of photon energy
Starting with Darwin width in the energy axis
)(02 hklhkl dfdEE
∝Δ
−=Δ
λλ
0
0.2
0.4
0.6
0.8
1
-5 -4 -3 -2 -1 0 1 2 3 4 5
10 keV30 keV
Ref
lect
ivity
2(x10-4)
1.4x10-4
ΔE/E
e.g. for Si 111 refl. DCM caseNote relative energy width is constant.
B2sin θ
χhrEE
≈Δ
Neglecting anomalous scattering factor f’
)(02 hklhr dfλχ ∝
22
B2
4
sin
λχ
θχ
λλ
hrhkl
hr
d
EE
=
≈Δ
−=Δ
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Effective band width (Integrated intensity)
∫=Δ dWWREE hr 2
B2 )(sin2 θ
χ
0
2
4
6
8
10
12
14
0 20 40 60 80 100Photon energy (keV)
Effe
ctiv
e ba
nd w
idth
Si 111 refl.
Si 311 refl.
Si 511 refl., Si 333 refl.
(x10-5)
For double-crystal monochromator
When you need flux Lower order (Si 111 refl.,..)
When you need resolution Higher order (Si 311, Si 511 refl,..)
Effective band-width is obtained
by integration of reflection curve.
= ~2
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Photon flux at undulator beamline
We can obtain photon flux of 1013~1014 ph/s/100 mA/mm2 using standard undulator sources and Si 111 reflections at SPring-8 beamlines.
1010
1011
1012
1013
1014
1015
1016
0 10 20 30 40 50Photon energy (keV)
Pho
ton
flux
(ph/
s/10
0 m
A) (a) total flux
(c)
(d)
(b) partial flux
(a) Total flux @ 0.1% b.w.(b) After frontend slit
1×1 mm2 @30 m(c) Si 111 refl. @10 keV
Effective b.w. = 1.3x10-4(d) 3rd harmonics @30 keV
Effective b.w. = 8.0x10-6
Higher harmonics elimination more mirror or detuning of DCM
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Double-crystal monochromator
Fixed-exit operation for usability at experimental station.
Choose suitable mechanism for energy range(Bragg angle range).
Precision, stability, rigidity,...
Offset h
y θB
O
A B
z
1st crystal
2nd crystal
θBθB
Exit beam B
hyθsin2
AB ==
B
hzθcos2
OB ==
Fixed-exit operation using rotation (θ) + two translation mechanism
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e.g. Double-crystal monochromator
θ-stage
Translation stage
1st crystal
2nd crystal
θ-stage
y
h
SPring-8 BL15XU
KEK-PF BL-4CMatsushita et al., NIM A246 (1986)
θ stage
1st crystal2nd crystal
θ rotation centerY1 stage
Z-cam stage
SPring-8 std. DCMYabashi et al., Proc. SPIE 3773, 2 (1999)
θ1 + translation + θ2 computer link
θ + two translation (2 cams)
θ + two translation (1 cam)
h= 25 mm, θB= 5~70°Offset h= 30 mm
θB =3~27º for higher energy range
h= 100 mm,
θB= 5.7~72°(for lower energy range)
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Crystal cooling
熱伝達
Qin T1
T0
Radiation & convection
Heat conduction in crystalHeat transfer
to coolant/holder Coolant/holder
Crystal
Why crystal cooling?Qin (Heat load by SR) = Qout (Cooling + Radiation,..)
with temperature rise ΔTαΔT = Δd (d-spacing change)
α: thermal expansion coefficientor Δθ (bump of lattice due to heat load)
Miss-matching between 1st and 2nd crystals occurs: Thermal drift, loss of intensity, broadening of beam, loss of brightnessMelting or limit of thermal strain Broken !
Solutions:(S-1) κ/α Larger(S-2) Contact area between crystal and coolant/holder
larger(S-3) Irradiation area Larger,
and power density smaller
Figure of meritSilicon Silicon Diamond300 K 80 K 300 K
κ (W/m/K) 150 1000 2000α (1/K) 2.5x10-6 -5x10-7 1x10-6
κ/α x106 60 2000 2000
We must consider:- Thermal expansion of crystal: α,- Thermal conductivity in crystal: κ,- Heat transfer to coolant and crystal holder.
Figure of merit of cooling:Good for silicon (80 k)
and diamond (300 K)
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Crystal cooling at SPring-8
Linear undulator, N= 140, λu= 32 mm
Power & power density: 300~500 W , 300~500 W/mm2
a) Direct cooling of silicon pin-postcrystal – (S2) & (S3)
b) Silicon cryogenic cooling - (S1)
c) IIa diamond with indirect water cooling - (S1)
0.6 mm
0.6 mm
0.5 mm
0.2 mm
Water flow
Water flow
X-rays
O-ring
Si-Au-Si bonding
Power & power density:
~100 W, ~1 W/mm2
Fin crystal direct-cooling - (S2)
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Example of x-ray beamline- SPring-8 case -
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XAFS & single crystal diffraction
- Bending magnet- Collimator mirror, + DCM,+ refocusing mirror
Roller
ShaftLink
Motor
(a)
(b)
Bellows
x
yδ
Beamline center
Collimatormirror
Double-crystalmonochromator
Gammastopper
Downstreamshutter
G1-G3: Gear box
Refocusingmirror
J1-J6: Jack
Fixed point
Ideal reflection axis
(0, h)
(x0, y0)h-y0
J1 J2 J3 J4 J5 J6G1 G2 G3
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Protein crystallography
- Bending magnet- DCM + focusing mirror
Focusing mirror(Vertical deflection)
Double-crystalmonochromator
Shielded tube
Optics hutch with standard components
Experimental hutch
Distance from the source50 m30 m 40 m
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High resolution inelastic scattering- Undulator- DCM + back-reflection monochromator & analyzer (w/ ~meV resolution)
Double-crystalmonochromator
Downstream shutter 1
Dual movableend-stopper
Experimental hutch 3(Back scattering hutch)
Experimental hutch 4(Analyzer hutch)
Experimentalhutch 2
Experimentalhutch 1
Optics hutch
Downstream shutter 2(Dual shutter)
Si 111 double-crystal beam displacerFocusing mirror
Downstream shutter 3 Back scattering
monochromator
Shielded beam ductSample position
Inclination stage
Distance from the source60 m30 m 40 m 50 m 70 m 80 m
5
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200-m-long beamline
- Bending magnet- DCM
Biomedical imaging centerExperimental hutch 2 and 3
Distance from the source220 m200 m180 m160 m140 m120 m
120 m100 m80 m60 m40 m
Dry pump
Dry pump
Beam monitor andgate valve
Roots pump with dry pump
Arcade400-mm-diameter shielded beam duct
Front end
Experimental hutch 1
Storage ring building
Optics hutch with standard transport channel and optics
300-mm-wide beam at end-station
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SummaryKey issues on the x-ray monochromator were shown,
introducing the dynamical x-ray diffraction for large & perfect crystal,
w/ several important points:
1) Total reflection occurs at the gap between dispersion surfaces.
2) Normalized deviation parameter W is related to the gap.
3) W is parameter of angular deviation and energy (wavelength) deviation.
It gives DuMond diagram as a band of |W|
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Text books following Laue’s dynamical theory
Ergebnisse der Exakt Naturwiss.
10 (1931) 133-158.
R. W. James
“The Dynamical Theory of X-Ray Diffraction”
Solod State Physics 15, (1963) 53-220.
Dover (1945)
Oxford (2001)
B. W. Batterman & H. Cole
“Dynamical Diffraction of X-Rays by Perfect Crystals”
Rev. Modern Phys. 36,
(1964) 681-717.Springer (2004)
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References
For monochromator[1] T. Matsushita & H. Hashizume,
Handbook on Synchrotron Radiation Vol. 1,
North-Holland (1983).
[2] Y. Shvyd’ko, Springer (2004), for high energy resolution
For atomic scattering factorFor f0
[3] International Tables for X-ray Crystallography (IUCr).[4] Hubbell et al.: J. Phys. Chem. Ref. Data Vol. 4, No. 3, 1975.For anomalous scattering factor f’, f”
[5] S. Sasaki, KEK report 88-14 (1989),[6] Tables of LBNL (B. L. Henke et al.),
http://henke.lbl.gov/optical_constants/index.html,[7] Tables of NIST,
http://physics.nist.gov/PhysRefData/FFast/html/form.htm
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Thanks to:
H. Kitamura, T. Tanaka, S. Takahashi, K. Takeshita,
N. Nariyama, Y. Asano, H. Ohashi, T. Mochizuki,
M. Yabashi, H. Yamazaki, K. Tamasaku, A. Baron,
M. Suzuki, T. Uruga, T. Matsushita, T. Ohata,
Y. Furukawa, and T. Ishikawa
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Thank you for your attention.